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Mid-infrared Extinction toward the Galactic Center

  • Authors: Sebastiano D. von Fellenberg, Joseph M. Michail, S. P. Willner, Braden Seefeldt-Gail, Tamojeet Roychowdhury, Macarena Garcia Marin, Giovanni G. Fazio, Nicole M. Ford, Daryl Haggard, Joseph L. Hora, Howard A. Smith, Zach Sumners, Gunther Witzel

Sebastiano D. von Fellenberg et al 2025 The Astrophysical Journal 995 .

  • Provider: AAS Journals

Caption: Figure 8.

Spatial variation of the line-derived extinction values for the 5.129 μm and 5.908 μm hydrogen recombination lines. The color bar shows the relative extinction measurements from the line ratios (A5.129/7.46 and A5.908/7.46) after they were converted to absolute extinction values by adding A7.46 = 0.64 mag derived from the Mini-spiral extinction measurement (Section 4.2). The white cross shows the approximate location of Sgr A*, and the lighter patches illustrate the two aperture masks used to obtain the line measurements in Figure 7. The rightmost panel shows the K-band extinction map derived from stellar colors (R. Schödel et al. 2010). The K band has higher absolute extinction (﹩{\left\langle A\right\rangle }_{2.16}\approx 2.4\,{\rm{mag}}﹩) but shows spatial variations similar to the MIR.

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